Journal
PHYSICAL REVIEW LETTERS
Volume 106, Issue 14, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.106.141101
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Funding
- U.S. NSF-Office of Polar Programs
- U.S. NSF-Physics Division
- University of Wisconsin Alumni Research Foundation
- GLOW and OSG grids
- U.S. DOE
- NERSCC
- LONI grid
- NSERC, Canada
- Swedish Research Council
- Swedish Polar Research Secretariat
- SNIC
- K. and A. Wallenberg Foundation, Sweden
- German Ministry for Education and Research
- Deutsche Forschungsgemeinschaft
- FSR
- FWO Odysseus
- IWT
- BELSPO, Belgium
- Marsden Fund, New Zealand
- JSPS, Japan
- SNSF, Switzerland
- EU
- Capes Foundation, Brazil
- NSF GRFP
- STFC [ST/J000507/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/J000507/1] Funding Source: researchfish
- Direct For Mathematical & Physical Scien
- Division Of Physics [0969661, 0856253, 757155] Funding Source: National Science Foundation
- Division Of Physics
- Direct For Mathematical & Physical Scien [0855486, 757759, 969061] Funding Source: National Science Foundation
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IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10(18) eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from p gamma interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence.
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